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Theory Tested by Means of the StarsThe viability of the solar alpha-omega dynamo model was studied through examination of extreme stellar cases expected to show specific types of deviation from solar behavior. Observational data was taken from studies of main sequence stars with shallow convective zones, fully convective M-dwarfs, and a Pleiades X-ray survey.
Document ID
19850009461
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Golub, L. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Date Acquired
August 12, 2013
Publication Date
January 1, 1985
Publication Information
Publication: NASA. Goddard Space Flight Center The Origin of Nonradiative Heating(Momentum in Hot Stars
Subject Category
Astronomy
Accession Number
85N17770
Funding Number(s)
CONTRACT_GRANT: NAGW-112
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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IDRelationTitle19850009446Collected WorksThe Origin of Nonradiative Heating/momentum in Hot Stars
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